Astronomy and Astrophysics – Astronomy
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.2106r&link_type=abstract
American Astronomical Society, SPD meeting #42, #21.06; Bulletin of the American Astronomical Society, Vol. 43, 2011
Astronomy and Astrophysics
Astronomy
Scientific paper
The thermal distribution of plasma in solar flares has been studied extensively and yet, remains evasive. Using the revolutionary spatial resolution and cadence of SDO/AIA, we analyze diffraction and dispersion effects out to more than 40 orders. Comparing the dispersion patterns to spectral results from SDO/EVE and RHESSI, and synthetic spectra from CHIANTI, we identify the distribution of plasma temperatures in a compact flaring loop with 12 second cadence. Unlike traditional spectroscopy, the high cadence of the AIA observations allow us to capture the highly dynamic nature of these eruptions with no compromise for spatial resolution or cadence.
Krucker Sa"m
Raftery Claire
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